to fund activities during Phase 1 of the Cosmic Axion Spin Precession Experiment (CASPEr), a search for ultra-light dark matter particles such as axions and dark photons

to support a workshop on precision measurement devices to study high energy physics in laboratory-scale experiments

for the acquisition and installation of an oxygen isotope ratio mass spectrometer system

for the optimization of a single-beam optically-levitated microsphere force-sensor for short-distance gravity experiments

for equipment and initial development of the Dark Matter Radio search for ultra-light axions and hidden photons

for the Physics and Astronomy Leadership Council

for the construction and operation of the Phase I Dark Matter Radio experiment

to support the inaugural Global Energy Forum at Stanford University

for studying how AMO physics can inform the development of gravity theories

for the Physics and Astronomy Leadership Council

to search for and characterize closely-separated binary systems of super massive black holes

for research on the formation and evolution of gas giant planets

for Unsolved Problems in Astrophysics – Bridging Theory and Observations of the Stellar Life Cycle

to retrieve and analyze microbes from atop Earth’s largest tropical glacier

for #BlackInAstro

for modeling chemistry, heat transfer, and material fluxes at the sea floor of Waterworld oceans.

to support the development of a comprehensive proxy-focused model of how marine sediment cores accumulate and change over millennial time scales to form the observed geological record

to support the development and application of data assimilation techniques in paleoclimate deep time

for a week-long workshop introducing participants to numerical modeling of the Earth’s climate and environmental systems

to support the development of novel algorithms and computational tools for high precision radial velocity measurements in the near-infrared wavelengths

for engineering analysis, instrumentation upgrades, and logistics planning for a network of glacier monitoring sensors in Greenland

for the 2018 Emerging Researchers in Exoplanet Science Symposium

to support the development of a new computational and statistical framework for discovering and characterizing low-mass exoplanets using upcoming extremely precise spectrographs

for the establishment of the Mercedes Richards Career Development Professorship endowment

for the Emerging Researchers in Exoplanet Science Symposium VII

for the 2024 Order of the Octopus SETI Conference

to develop technology and techniques that will advance the state-of-the-art in direct exoplanet imaging

for the 51 Pegasi b Fellowship

for hydroclimate research using clumped isotope analysis

for the development of more sophisticated methodologies and computational tools for measuring the stellar orbits of stars near supermassive black holes to further our understanding of the physics associated with black holes

for the Physics and Astronomy Leadership Council

to plan for growth within the activities of the Galactic Center Orbits Initiative

for instrumentation and its application to carbonate clumped isotope analysis

for the Keck Planet Finder Community Cadence initiative

to investigate the origin of small planets with the Keck Planet Finder

for clumped isotope paleo-hydroclimate analysis

to support the Particle Cosmology Southwest Workshop

to endow the Andrea M. Ghez Centennial Term Chair in Astronomy and Astrophysics

to develop novel computational modeling tools to test general relativity at the event horizon of a supermassive black hole

to apply astronomical image processing to fluorescence microscopy imagery

to fund Boston University’s activities during Phase 1 of the Cosmic Axion Spin Precession Experiment (CASPEr), a search for ultra-light dark matter particles such as axions and dark photons

to apply astronomical image processing to fluorescence microscopy imagery

for research into Solar System fundamental frequencies, Earth precession frequency, and lunar periodicities

for studying Solar System dynamics through the analysis of Triassic and Jurassic geological records

for analyzing data from the Gattini-IR wide-field infrared imager

for the creation of the paleopCO2.org website and associated tools and content

to study the impact of atmospheric variability and shallow hydrology on the flow dynamics and mass budget of the Helheim Glacier

to collect in situ measurements of ice-shelf rivers and estuaries

to bridge a flight delay for the GAPS experiment

for the development and application of hydrology models for snow, firn, and subglacial flows at Helheim Glacier